New Northern Horizons

SHO2int3 (Large)

Having past the Autumn Equinox I’ve moved the observatory back to its main location on the patio looking south for the winter but not before a final look at the northern sky from the newly established Shed Observatory situated at the end of the garden.  After setting up The Shed in mid-May I have had a productive and very enjoyable time imaging and looking at the northern night sky properly for the first time.  My objective has been to learn more about this part of the sky and bag as many northern DSO classics as possible during the limited darkness available at this time of the year.  Furthermore, I set out to determine optimum imaging parameters for these objects in preparation for more extensive sessions at the same time next year.

Altogether I managed six targets with some good results, three of which have already been posted here: M81 Bodes & M82 Cigar galaxies, IC 1396 Elephant’s Trunk Nebula and IC 1805 the Heart Nebula. Whilst the new Shed Observatory provided a good view of much of the north sky, I did cut corners with the set-up and as a result guiding was not always at its best, sometimes with an impact on quality.  This has been a period of experimentation but now I know this location works, next time I’ll pay more attention to these matters.  In addition to the aforementioned objects I was also able to image three others, with mixed results.

I came across NGC 7822 soon after moving to the new Shed Observatory site whilst investigating the imaging possibilities from this location.  This complex emission nebula appears to be overlooked by many astrophotographers, though judging from the images that are available it can be quite a spectacular target, providing great promise in narrowband wavelengths when using the right equipment.  Whilst the main Ha image looked promising (below), sadly on this occasion the SHO & HOO images lack detail and colour; on reflection the focus looks a bit suspect too!

IMAGING DETAILS
Object NGC 7822
Constellation Cepheus
Distance 2,900 light-years
Size 100’   
Apparent Magnitude +18.3
 
Scope  William Optics GT81 + Focal Reducer FL 382mm  f4.72
Mount SW AZ-EQ6 GT + EQASCOM computer control
Guiding William Optics 50mm guide scope
  + Starlight Xpress Lodestar X2 guide camera & PHD2 control
Camera ZWO1600MM-Cool (mono)   CMOS sensor
  FOV 2.65o x 2.0o Resolution 2.05”/pix  Max. size 4,656 x 3,520 pix   
EFW ZWOx8 + ZWO LRGB & Ha OIII SII 7nm filters 
Capture & Processing Astro Photography Tool + PS2,  Deep Sky Stacker & Photoshop CS2, HLVG
Image Location              & Orientation Centre  RA 00:02:35     DEC 67:13:55                     

North Sky: Top Left = North  Top Right = East  

Exposures 20 x 180 sec Ha + 10×180 sec OIII & SII  (Total time: 120 minutes)   
  @ 300 Gain   50 Offset @ -20oC    
Calibration 5 x 300 sec Darks  20 x 1/4000 sec Bias  10 x Flats Ha-OIII-SII  @ ADU 25,000  
Location & Darkness Fairvale Observatory  South – Redhill – Surrey – UK        Typically Bortle 5
Date & Time 20th May 2018 @ +00.00h  
Weather Approx. <12oC   RH 70%

Once astronomical darkness was re-established in late July I soon returned to the northern sky thereafter.  After a gap of more than 2-months since my previous session in May, the north sky now provided other new opportunities, principal of which were the Heart Nebula and Soul Nebula.  Given their size and my field-of-view these objects need to be imaged separately and after a good result with the Heart Nebula, I was soon also able to tackle the nearby Soul Nebula.  However, this time the guiding was at first very poor and I decided to use the PHD2 Guiding Assistant to help correct the problem.  The new settings recommended by the Assistant made a big difference to the guiding but unfortunately I then overlooked that the consequence of running the process had changed the previous image framing of the object.  As a result of this the lower section of the nebula was no longer within the field-of-view and subsequently lost in the final image – oh well lesson learned for another day.

HaHOO crop (Large)

IMAGING DETAILS – Soul Nebula HaHOO (above) 
Object Soul Nebula IC 1848   (Westerhout-5)
Constellation Cassiopeia
Distance 6,500 light-years
Size 150’ x 75’  or 100 light-years
Apparent Magnitude +18.3
 
Scope  William Optics GT81 + Focal Reducer FL 382mm  f4.72
Mount SW AZ-EQ6 GT + EQASCOM computer control
Guiding William Optics 50mm guide scope
  + Starlight Xpress Lodestar X2 guide camera & PHD2 control
Camera ZWO1600MM-Cool (mono)   CMOS sensor
  FOV 2.65o x 2.0o Resolution 2.05”/pix  Max. size 4,656 x 3,520 pix   
EFW ZWOx8 + ZWO LRGB & Ha OIII SII 7nm filters 
Capture & Processing Astro Photography Tool + PS2,  Deep Sky Stacker & Photoshop CS2, HLVG
Image Location              & Orientation Centre  RA 02:52:25    DEC 60:01:35                     

Top  Left North  Top Right = East   Bottom Right = South   Bottom Left = West      

Exposures 20 x 300 sec Ha + 10×300 sec OIII  (Total time: 150 minutes)   
  @ 139 Gain   21  Offset @ -20oC    
Calibration 5 x 300 sec Darks  20 x 1/4000 sec Bias  10 x Flats Ha-OIII-SII  @ ADU 25,000  
Location & Darkness Fairvale Observatory – Redhill – Surrey – UK        Typically Bortle 5
Date & Time 2nd September 2018 @ +00.20h  
Weather Approx. 12oC   RH <=95%

Finally I was surprised and pleased to discover that with the early evening darkness now available in September, I might be able to image the strange but beautiful Bubble Nebula NGC 7635.  Being very high in the sky at this time, the challenge was to track the object for as long as possible before at about 1.00 a.m. it disappears overhead behind the high garden hedge located immediately adjacent to the telescope location.  I managed, just about, and was very happy to see the ‘bubble’ in the middle of the resulting image. The enigmatic bubble is created by a stellar wind from a massive, hot central star (SAO 20575) which excites the nebula and causes it to glow.  Whilst the central Bubble Nebula is undoubtedly the star of the show, this region of the sky and resulting picture holds great promise to image other objects on another occasion, notably the open cluster M51 just below and to the left of the Bubble and the Lobster Claw Nebula SH2-157 in the top-right corner.

Ha2A (Large)

 

Claw2

IMAGING DETAILS: Bubble Nebula – Ha above, SHO top of page 
Object Bubble Nebula NGC 7635
Constellation Cassiopeia
Distance 7,100 light-years
Size 15’ x 8’  (Bubble 7 light-years)
Apparent Magnitude +10.0
 
Scope  William Optics GT81 + Focal Reducer FL 382mm  f4.72
Mount SW AZ-EQ6 GT + EQASCOM computer control
Guiding William Optics 50mm guide scope
  + Starlight Xpress Lodestar X2 guide camera & PHD2 control
Camera ZWO1600MM-Cool (mono)   CMOS sensor
  FOV 2.65o x 2.0o Resolution 2.05”/pix Max. size 4,656 x 3,520 pix   
EFW ZWOx8 + ZWO LRGB & Ha OIII SII 7nm filters 
Capture & Processing Astro Photography Tool + PS2,  Deep Sky Stacker & Photoshop CS2, HLVG
Image Location              & Orientation Centre  RA 23:21:27    DEC 61:06:52                     

Top = north  Right = East   Bottom = South  Left = West 

Exposures 15 x 300 sec Ha + 10×300 sec OIII & SII  (Total time: 175 minutes)   
  @ 139 Gain   21  Offset @ -20oC    
Calibration 5 x 300 sec Darks  20 x 1/4000 sec Bias  10 x Flats Ha-OIII-SII  @ ADU 25,000  
Location & Darkness Fairvale Observatory – Redhill – Surrey – UK        Typically Bortle 5
Date & Time 3rd September 2018 @ +21.45h  
Weather Approx. 15oC   RH >=70%

My time at the end of the garden this summer at the Shed Observatory has been a great success, made all the better by a prolonged period of warm weather.  I am confident that with more attention to the set-up, better guiding and longer integration times, next year will be even better and I’m already looking forwards to revisiting this year’s new horizons in the north sky in 2019.

North Sky summer Objects

North Sky Imaged Objects May to September 2018

Heart Of Darkness

HHOO hlvg (Large)

Aside from all the paraphernalia required for astrophotography, two other critical items are essential to start imaging: clear skies and darkness.  This year astronomical darkness ceased on 25th May at Fairvale Observatory and remained absent for the next 8-weeks  whilst Earth performed its annual summer gyration about the Sun, culminating on 21st June with the solstice.  As a result this period is typically quite a barren time for astronomers, especially for those in the higher latitudes where the sun does not set for the entire 24-hour day.  Some options during this time are:  give up, stop imaging and use the time to sort out equipment, if you have the right equipment change to solar astronomy or just enjoy what happens to be about in the less than dark sky.  This year I chose the latter, during what has been a very hot summer, often with continuously clear skies for days-on-end.

Planets June 2018

From the early evening we’ve been treated to views of all the planets of the Solar System, as during the short nights one-by-one they transited along the ecliptic, though were relatively low in the sky seen from the UK.  In order of appearance, the main show (see above) each night has been that of Jupiter, followed by Saturn and finally at about 2.00 a.m. (June) Mars – which this year was an unusually large, unusually bright  red disc as it reached its closest orbit relative to Earth for almost 60,000 years – all of which could be clearly seen with the naked eye.  Unable to sleep in the hot weather, night after night I was able to view and sometimes imaged the aforesaid planets with a DSLR camera as they moved across the night sky.

Shortly after darkness started to return on 20th July came two further special events.  First on 27th July a lunar eclipse, that despite all the previous clear nights was ironically obscured by cloud cover over most of the UK!  Fortunately, clear skies returned for 13th August and the annual Perseids meteor shower, which on this occasion produced some of the best meteor trails I have personally experienced.

And so, with astronomical darkness back and the chance to return to the recently established Fairvale Observatory South AKA The Shed Observatory, it was time to resume my hitherto brief imaging experience of the northern sky again.  As a newcomer to this part of the night sky there were considerable new imaging possibilities to explore but only one I now wanted to capture – the Heart Nebula or IC 1805 (also known as the Running Dog Nebula when viewed from a different angle).

Heart-and-Soul-location The Heart and nearby Soul Nebula are situated in a busy region of the sky (see above – from Wikisky), which also contains seven open clusters of young stars, as well as the Pacman Nebula and galaxies of Maffei 1 & 2 and M31 Andromeda.  The discovery of a bright fish-shaped HII object – known as the Fishhead Nebula IC 1795 or NGC 896 at the edge of the main object – preceded that of the Heart Nebula itself in 1787 by William Herschel.  The Heart Nebula has a red glow, a result of intense radiation emanating from a small cluster of large, hot, young (1.5 My) bright-blue stars at the centre known as Melotte-15.  The stellar wind and stream of charged particles that flow out from these newborn stars then creates the characteristic heart-shape of the nebula from the stellar dust and hydrogen gas clouds.

Picture saved with settings embedded.

Located in the Perseus arm of the Milky Way in the Cassiopeia constellation, this large emission nebula is an excellent object for narrowband imaging at all wavelengths and is also well framed in the field-of-view of my telescope-camera combination; the images presented here are rotated 180 degrees to achieve the correct orientation to see the heart shape, with the Fishhead Nebula located in the bottom right corner.  Not surprisingly this large HII object produces strong Ha subs, which make a pleasing stand-alone image (above section). But the OIII and especially SII wavelengths are also very good, resulting in very good HHOO bi-colour (top-of-the-page) and SHO (below) images too.

SHO end3Final (Large)

The limited time I’ve had to image the northern sky for the first time this year has already proved to be exciting and bodes well for the future.  On this occasion I’ve been very pleased with my first imaging results of the Heart Nebula, which is a superb object for my equipment and am sure to return next year given suitably clear skies and, of course, darkness.

IMAGING DETAILS
Object Heart Nebula IC 1805    AKA Running Dog Nebula   Sharpless 2-190
Constellation Cassiopeia
Distance 7,500 light-years
Size 150’ x 150’  =  2.5o or 200 light-years
Apparent Magnitude +18.3
 
Scope  William Optics GT81 + Focal Reducer FL 382mm  f4.72
Mount SW AZ-EQ6 GT + EQASCOM computer control
Guiding William Optics 50mm guide scope
  + Starlight Xpress Lodestar X2 guide camera & PHD2 control
Camera ZWO1600MM-Cool (mono)   CMOS sensor
  FOV 2.65o x 2.0o Resolution 2.05”/pix  Max. image size 4,656 x 3,520 pix   
EFW ZWOx8 + ZWO LRGB & Ha OIII SII 7nm filters 
Capture & Processing Astro Photography Tool + PS2,  Deep Sky Stacker & Photoshop CS2, HLVG
Image Location             & Orientation Centre  RA 02:33:09    DEC 61:24:23 

Top = South   Right = West   Bottom = North   Left = East  

Exposures 20 x 300 sec Ha + 10×300 sec OIII & SII  (Total time: 200 minutes)   
  @ 139 Gain   21  Offset @ -20oC    
Calibration 5 x 300 sec Darks  20 x 1/4000 sec Bias  10 x Flats Ha-OIII-SII  @ ADU 25,000  
Location & Darkness Fairvale Observatory – Redhill – Surrey – UK        Typically Bortle 5
Date & Time 16th & 17th  August 2018 @ +23.30h  
Weather Approx. 12oC   RH <=95%

 

Jumbo Joy

Picture saved with settings embedded.

After recently establishing Fairvale Observatory South AKA “The Shed” and dealt with some expected and unexpected problems, I was able to turn my attention to the object of my desire in this hitherto inaccessible part of the northern night sky.  With the summer solstice approaching I had originally planned on imaging this astrophotographers’ favourite later in the year but I couldn’t resist an early look.  A few nights after finishing Bodes galaxy from my new, northward looking location, I therefore swung the scope across the Meridian to the north east in order to obtain a few subs of this object just to see: (a) what it might look like with my equipment (b) bearing in mind the previous objective, to assess the best framing and (c) just for the fun of it, and was not disappointed!

RGB XXX Final (Large)The aforesaid object of interest was the Elephant’s Trunk Nebula or IC 1396, a very large emission nebula, which in narrowband shows wonderful colour and detail (HaSHO above).  IC 1396 consists of glowing gas illuminated by an open star cluster, broken up by intervening lanes of dark interstellar dust clouds.  The ‘trunk’ itself, designated IC 1396A, is the long dark area protruding from the lower edge of the image, spectacularly illuminated from behind by a bright star forming region; the image has been rotated 180o from its natural position.  Top right on the edge is the red supergiant Mu Cephei or Herschel’s Garnet Star, one of the largest and brightest known stars in the Milky Way, which in the position of the Sun would extend out to Saturn’s orbit!

HHOO (Large)

The large IC 1396 nebula will not fit my field-of-view but with some judicious framing, using the Garnet Star as a marker and helped by a few previously taken test subs, I achieved a pleasing composition with the aforesaid trunk and nearby billowing dark clouds well placed (HaOIIIOIII bicolour image above).  Whilst I am pleased with my first attempt at the Elephant’s Trunk, the colour could be better and is too noisy – a consequence of too little integration time and high gain setting.  Having had success before using similar settings for Ha-type features like the Rosette Nebula, I was a little surprised by this outcome but it just goes to show that each object is different.  Notwithstanding, the Ha version is – I think – very promising (top of the page) but obviously there is too little OIII and SII in the composite wavelength images.

RGB XXX Final Crop (Medium)

I used to live and have worked all over Africa but this is a very different type of elephant to what I have met before (the “trunk” HaSHO above).  It forms an exciting imaging subject at this time of the year, made all the more rewarding being one of my first serious attempts to image the north sky.  I hope to return to this object in a couple of months when astronomical darkness has resumed but in the meantime the Jumbo of the night sky has been a real joy on my first encounter.

Elephant Location Crop

IMAGING DETAILS
Object Elephant’s Trunk Nebula   IC 1396   
Constellation Cepheus
Distance 2,400 light-years
Size 5o or “Trunk” only approx.. 45’   
Apparent Magnitude +3.5 to +5.7
 
Scope  William Optics GT81 + Focal Reducer FL 382mm  f4.72
Mount SW AZ-EQ6 GT + EQASCOM computer control
Guiding William Optics 50mm guide scope
  + Starlight Xpress Lodestar X2 guide camera & PHD2 control
Camera ZWO1600MM-Cool (mono)   CMOS sensor
  FOV 2.65o x 2.0o Resolution 2.05”/pix  Max. image size 4,656 x 3,520 pix   
EFW ZWOx8 + ZWO LRGB & Ha OIII SII 7nm filters 
Capture & Processing Astro Photography Tool + PS2,  Deep Sky Stacker & Photoshop CS2
Image Location Centre  RA 21:38:37    DEC 57:30:16  
Exposures 12 x 300 sec Ha + 6 x300 sec OIII & SII  (Total time: 120 minutes)   
  @ 300 Gain   50 Offset @ -20oC    
Calibration 5 x 300sec Darks  20 x 1/4000 sec Bias  10 x  Ha + OIII + SII  Flats @ ADU 25,000  
Location & Darkness Fairvale Observatory – Redhill – Surrey – UK        Typically Bortle 5
Date & Time 22nd May 2018  @ midnight

Boreal Breakthrough

 

M81 LRGB Final HLVG

I have often written about imaging difficulties here at Fairvale Observatory, which apart from overflying aircraft from Gatwick and Heathrow airports, 24/7 helicopters from Redhill aerodrome and general light pollution, also consists of numerous sightline obstructions in the form of large trees to the east and south, high garden hedges and the complete obstruction of the north sky by my house!  I have toyed with the idea of moving onto the lawn so as to look back northwards over the house but was concerned by all the faffing about to get the equipment down and back up a flight of steps, as well as added complications with equipment control and dew problems; I concede that many do operate successfully in this way but with plenty of other problems to cope with, I like my hobby to be as easy and convenient as possible.

Last year I enjoyed working outside during the summer months – notwithstanding the lack of darkness during much of this period – and therefore over the past winter finally considered how such a garden-based set-up could be achieved, primarily for use between May and September.  The resulting Plan-A was to place three paving stones within the lawn to support the tripod and run a USB-cable back to the house for control.  However, after recently expanding a small paved area outside the shed at the end of the garden and looking at the potential sightlines from this location, it was obvious that a Plan-B set-up here could also work.  Whilst not quite as good viewing angles as the original location, there are a number of other worthwhile benefits:

  • Being off the lawn on paving it seemed likely that dew could be less of a problem;
  • Working on the paving around the mount would be more convenient and dry;
  • By clearing out the adjacent shed it could be used as a dry location from which to control the equipment.

And so early in May I set about establishing Plan-B and soon afterwards putting it to work.

Pan1 Comp (Medium)

The view from the shed looking northwards is surprisingly quite good (see above) and I don’t know why I hadn’t considered this before. There are a few large trees to the north east, a high hedge along the western boundary and of course my house is still somewhat in the way but altogether it’s not too bad and for the first time I have a clear view of Polaris, as well as a whole new plethora of imaging targets!  Whilst this direction looks directly towards south London, being on the southern slope of the Greensand Ridge the worst of the city’s glow is fortunately obscured by the hill.  Furthermore, it is ironic that my house and the hedges also provide considerable protection from the local street lights, which I’m pleased to say are now turned off after midnight anyway.

Set-up

Local equipment layout the same as previously

I cut-back some of the adjacent vegetation to improve sightlines and ran a power cable from the house to the shed otherwise it’s exactly the same set-up which was being used at the main, south looking location on the patio by the house.  I looked into WiFi-control of the equipment but from the experience of others concluded it could be unreliable and instead considered using Teamviewer software via a USB Cat-5 repeater cable from the mount / shed computer to a second computer in the house.  However, given the distance of some 30 metres I finally decided to adopt a more robust LAN Cat-6 ethernet cable for this purpose. Unfortunately whilst this had worked successfully during testing in the house, I have so far been unable to get it to work outside and for now have had to operate the equipment from inside the shed, which has nonetheless proved to be a comfortable and effective alternative.

Being lazy and cautious about changing too much about the set-up, I levelled, aligned and reset the new location data of the tripod but kept all other settings the same for now.  I realise this is not ideal but initially just wanted to experience the new location and north sky to understand what was possible within the given field-of-view and identify any obvious problems.  Fortunately a settled period of good weather allowed me to try out the new location soon thereafter.

North Sky ViewX

White area shows optimum imaging area from Fairvale Observatory South – AKA ‘The Shed’

What I hadn’t expected on first use was that slewing and tracking would become more difficult and takes noticeably longer at higher latitudes, especially approaching Polaris.  Following subsequent enquiries and with some further thought it now makes sense.  At higher latitudes near and above about 70 degrees as the lines of Longitude are closer together, it makes the RA slew rate bigger and bigger the closer you get to the North Celestial Pole.  Of course the celestial pole is not coincident with the terrestrial pole, which means that those objects within the latitude of 90o minus the observer’s latitude – in my case this equals 39o – means that all those objects above 39o will be circumpolar from my point-of-view i.e. will rotate over the year around North Celestial Pole.  This is basic astronomy but hitherto I had not considered the implications for tracking and guiding before and will need to bear it in mind when selecting targets in the future.

M81 B (Large)

I had one particular target in mind but as it was only viable much later in the night, on this occasion I chose to start imaging the north sky for the first time with Bode’s Galaxy AKA M81 and the nearby Cigar Galaxy AKA M82; for comparison using low gain, long exposure on the first night (top of the page) and high gain, short exposure (below) on the following night.  Given the target’s DEC position of 70o I soon discovered the aforesaid tracking difficulties, which resulted in the RMS guiding error varying from 3’ to 20’ and deleterious consequences for the images!

 

Whilst I’m pleased with my very first north sky images, it is obvious I’ll need to return again with better guiding and much longer integration time.  On a positive note the general set-up worked very well and the shed provided an excellent place from which to operate the control and image capture equipment.  Furthermore, despite a few restrictions the overall view of the northern night sky is good and holds much promise for future, hitherto inaccessible imaging objects.  As a result of establishing this new site I intend to name the new north looking location Fairvale Observatory South or ‘The Shed Observatory’ (see mosaic above) and the principal, south looking location by the house Fairvale Observatory North or ‘The Patio Observatory’.  Altogether this marks a major breakthrough for my astronomy and I eagerly await the return of astronomical darkness on 20th July onward.

AstroNet ResultX

IMAGING DETAILS
Objects Bode’s Galaxy M81  &  Cigar Galaxy M82     
Constellation Ursa Major
Distance M81  11.8  &  M82  11.4 -12.4 million light-years
Size M81 26.9’ x 14.1’   &    M82 11.2’ x  4.3’
Apparent Magnitude M81 +8.0  &  M82 +8.4
 
Scope  William Optics GT81 + Focal Reducer FL 382mm  f4.72
Mount SW AZ-EQ6 GT + EQASCOM computer control
Guiding William Optics 50mm guide scope
  + Starlight Xpress Lodestar X2 guide camera & PHD2 control
Camera ZWO1600MM-Cool (mono)   CMOS sensor
  FOV 2.65o x 2.0o Resolution 2.05”/pix  Max. image size 4,656 x 3,520 pix   
EFW ZWOx8 + ZWO LRGB & Ha OIII SII 7nm filters 
Capture & Processing Astro Photography Tool + PS2,  Deep Sky Stacker & Photoshop CS2
Image Location Centre Image-B    RA 09:55:13.46    DEC 69:21:08.36  (19/0518) 
Exposures                       

                                       

                                         

A 18/05/18   10 x 180 sec L  + 5×180 sec RGB  (Total time: 75 minutes)    @ 139 Gain   21  Offset @ -20oC

B 19/05/18   45 x 60 sec L    + 15 x 60 sec RGB  (Total time: 90 minutes)    @ 300 Gain   50  Ofsett @ -20oC    

Calibration                    

                                        

A 15 x 180sec Darks  20 x 1/4000 sec Bias  10 x Flats LRGB  @ ADU 25,000  

B 15 x 60sec Darks     20 x 1/4000 sec Bias  10 x Flats LRGB  @ ADU 25,000  

Location & Darkness Fairvale Observatory South – Redhill – Surrey – UK       Typically Bortle 5
Date & Time (A)    18th  &   (B) 19th May 2018 @ +23.45h approx.

 

 

Star Struck

 

M13 LRGB F2 CROP (Large)

Of all the things I’ve discovered since taking up astronomy, perhaps it is the presence and nature of globular clusters that has most surprised me. Bound closely together by gravity, these massive spherical collections of stars orbit the galactic core perpendicular to its plane.  In the case of the Milky Way there are 150 globular clusters but they can be much larger in other galaxies, such as M87 which has some 13,000; clusters of clusters have also now been discovered in the Universe!  Typically each cluster might contain a few thousand or tens of thousands of stars, although in some cases they can be much larger.  Omega Centauri is the largest globular cluster in the Milky Way, being 150 light-years in diameter it contains 10 million stars; though clearly visible from Earth it can only be viewed from the Southern Hemisphere, which we unfortunately did not see when in New Zealand earlier this year.

MW &amp; globs

Despite all the advances being made in cosmology, the origin of globular clusters still seems to remain quite uncertain.  Characteristically the stars are all very old, typically in the region of 8 to 12-billion years and are of low metallicity i.e. they contain a low proportion of elements other than hydrogen and helium.  At least some, such as Alpha Centauri, are thought to have condensed from dwarf galaxies and such a process may currently be taking place within the large Magellanic Cloud – which we did see in New Zealand!  In other cases it is thought that the clusters have probably originated independently and were subsequently captured by the relevant galaxies.  However, their very old age – sometimes nearly as old as the universe itself – origin and relationship to galaxies remains intriguing.  For these and many other reasons I personally find globular clusters fascinating, probably more than any other astronomical feature, amazing as they too may be.

GlobsX

Globular Clusters May 2018: M3, M13 & M92 (red circles) + Others (yellow circles)

From time-to-time I’ve tried imaging various globular clusters but have not been satisfied with the outcome.  Now using guiding, plate solving and the high-resolution ZWO1600MM-Cool camera, it was time to give it another try this spring, when some of the best clusters are present in the northern night sky.

M3 LRGB Final (Large)

First up was M3 (Final image above), the very first Messier Object to be discovered by Charles Messier himself in 1764.  Consisting of 500,000 stars, between 8 and 11-billion years old and spanning some 220 light-years, M3 is one of the largest and brightest (absolute) globular clusters associated with the Milky Way – about 300,000 times brighter than our Sun.  It is noteworthy that the cluster contains some 274 variable stars, the highest number of any clusters, as well as a relatively high number of ‘blue stragglers’ – young main-sequence stars that appear to bluer and more luminous than the other stars in the cluster and are thought to be formed through stellar interaction of the older stars.

M3 LRGB Crop (Large)

With these attributes it is not surprising that M3 is considered a popular target in astrophotography (cropped image above), likely surpassed however by M13 AKA the Great Globular Cluster in Hercules (cropped image top-of-the-page), which conveniently follows M3 in the same area of the sky about 3-hours later (together with nearby the globular cluster M92).  And so having bagged M3 it was time to turn the telescope and camera towards M13 (Main image below).  Discovered by the eponymous Edmond Hailey in 1716 (he of Hailey’s Comet), seen from Earth M13 is slightly brighter than M3 with a wide range of star colours that certainly makes for an exciting image.  At 11.65 billion years old, M13 has been around almost three times as long as the planet Earth.

M13 LRGB Final (Large)

Since starting astrophotography I like to try my hand at imaging a globular cluster at least once each year but hitherto with disappointing results.  This time I’m pleased with the outcome, especially M13 which is surely one of the most magnificent objects in our night sky; as a bonus there are also a few galaxies in the background of both the M3 and M13 images too.  It is therefore fortunate that for those of us in the higher latitudes of the northern hemisphere the Great Globular Cluster in Hercules can be seen all-year round, though is at its highest and therefore best position between May and September – thereby inaccessible for the Kiwis who are instead compensated by Alpha Centauri!  I expect to be back again next year to marvel at these amazing and enigmatic objects, if not before.

M3 Location Crop

IMAGING DETAILS
Object M3    (NGC 5272)     
Constellation Canes Venatici
Distance 33.9 million light-years
Size 18.0’ or 220 light-years     
Apparent Magnitude +6.2
 
Scope  William Optics GT81 + Focal Reducer FL 382mm  f4.72
Mount SW AZ-EQ6 GT + EQASCOM computer control
Guiding William Optics 50mm guide scope
  + Starlight Xpress Lodestar X2 guide camera & PHD2 control
Camera ZWO1600MM-Cool (mono)   CMOS sensor
  FOV 2.65o x 2.0o Resolution 2.05”/pix  Max. image size 4,656 x 3,520 pix   
EFW ZWO x 8 + ZWO LRGB & Ha- OIII-SII 7nm filters 
Capture & Processing Astro Photography Tool + PS2,  Deep Sky Stacker & Photoshop CS2
Image Location Centre  RA 13:42:23     DEC 28:22:50  
Exposures 24 x 180 sec L + 10×180 sec RGB  (Total time: 162 minutes)   
  Unity @ 139 Gain   21  Offset @ -20oC    
Calibration 10 x 180sec Darks  20 x 1/4000 sec Bias  10 x Flats LRGB  @ ADU 25,000  
Location & Darkness Fairvale Observatory – Redhill – Surrey – UK        Typically Bortle 5
Date & Time 5th + 6th  May 2018 @ +23.00h

M13 Location Crop

IMAGING DETAILS
Object M13     (NGC 6205)
Constellation Hercules
Distance >=20,000 light-years
Size 20’  or 150 light-years
Apparent Magnitude +5.8
 
Scope  William Optics GT81 + Focal Reducer FL 382mm  f4.72
Mount SW AZ-EQ6 GT + EQASCOM computer control
Guiding William Optics 50mm guide scope
  + Starlight Xpress Lodestar X2 guide camera & PHD2 control
Camera ZWO1600MM-Cool (mono)   CMOS sensor
  FOV 2.65o x 2.0o Resolution 2.05”/pix  Max. image size 4,656 x 3,520 pix   
EFW ZWOx8 + ZWO LRGB & Ha OIII SII 7nm filters 
Capture & Processing Astro Photography Tool + PS2,  Deep Sky Stacker & Photoshop CS2
Image Location Centre  RA 12:39:59    DEC -11:37:20  
Exposures 20 x 180 sec L + 15×180 sec RGB  (Total time: 195 minutes)   
  @ Unity 139 Gain   21  Offset @ -20oC  USB 40 
Calibration 10 x 180sec Darks  20 x 1/4000 sec Bias  10 x Flats LRGB  @ ADU 25,000  
Location & Darkness Fairvale Observatory – Redhill – Surrey – UK        Typically Bortle 5
Date & Time 6th + 7th + 9th May 2018 @ +00.30h  

 

Chapeau!

LRGB GxC Crop-2 (Large)

 

I always had a general interest in astronomy but was eventually sparked into action after viewing Saturn through the Thompson 26 inch refractor at Herstmonceaux observatory in 2014.  The beauty of the planet and its unique rings is captivating and like many others it remains my favourite planet to this day.  One year on and looking further afield at Joan Genebriera’s Tacande Observatory on the island of La Palma, I discovered what is now  one of my very favourite Deep Sky Objects – M104 or the Sombrero Galaxy; until recently I used the resulting picture obtained whilst at La Palma as the main banner image for this website.  Though perhaps not as spectacular as the Orion Nebula or certain spiral galaxies, the sombrero-like galaxy (with a passing resemblance of a flying saucer too), is beguiling in its own unique way and ever since then I’ve been eager to return to The Hat and image it myself from home.

Chart_1.cdc3

However, imaging the Sombrero from the UK and especially at my location just south of London is quite another matter to La Palma.  Aside from light pollution, being at 51o north compared to 28o in La Palma, M104 is considerably lower in the sky when viewed from Fairvale Observatory in Redhill; at the time of imaging in early May it was about 26o above the southern horizon.  Furthermore, my sight lines are obscured on three sides by 15-foot hedges and directly south by two 45-foot conifers – see below SE to SW view of M104 imaging track at Fairvale Observatory.

M104 Track crop

As a result, only after it emerges from behind the western edge of the aforesaid conifers can M104 (just) be imaged, as it moves along the top of the hedge for just over an hour before disappearing from view once again.  Of course this is far from ideal but with my enthusiasm for the Sombrero, a high-resolution ZWO1600M-Cool camera and newly acquired ability to plate solve, I gave it a try over three consecutive nights.

 

RGB GxC crop (Large)

 

An unbarred spiral galaxy, the hallmark of M104 is its bright bulbous centre encircled by dark dust lanes, which when viewed from Earth tilted at just 6-degrees above the equatorial plane creates the appearance of a sombrero hat (see cropped image above).  With the much higher resolution of the Hubble telescope some 2,000 globular clusters have been identified with M104, ten-times that of the Milky Way.  In 1912 the galaxy was found to be moving away from Earth at 700 miles per second, providing an early indication that the Universe was in fact expanding in all directions.

All-in-all the Sombrero galaxy is a fascinating and unusual object, though small and all-in-all a challenging imaging target, especially seen from Fairvale Observatory.  Notwithstanding, at last I am very pleased to obtain my own exciting image of the Sombrero – chapeau!

M104 Location

IMAGING DETAILS
Object Sombrero Galaxy  M104     
Constellation Virgo
Distance 29 million light-years
Size 9’ x 4’  or  50,000 light-years
Apparent Magnitude +8.0
 
Scope  William Optics GT81 + Focal Reducer FL 382mm  f4.72
Mount SW AZ-EQ6 GT + EQASCOM computer control
Guiding William Optics 50mm guide scope
  + Starlight Xpress Lodestar X2 guide camera & PHD2 control
Camera ZWO1600MM-Cool (mono)   CMOS sensor
  FOV 2.65o x 2.0o Resolution 2.05”/pix  Max. image size 4,656 x 3,520 pix   
EFW ZWOx8 + ZWO LRGB & Ha OIII SII 7nm filters 
Capture & Processing Astro Photography Tool + PS2,  Deep Sky Stacker & Photoshop CS2
Image Position Centre  RA 12:39:59    DEC -11:37:20  
Exposures 25 x 180 sec L + 3x5x180 sec RGB  (Total time: 120 minutes)   
  @ 139 Gain   21  Offset @ -20oC    
Calibration 10 x 180sec Darks  20 x 1/4000 sec Bias  10 x Flats LRGB  @ ADU 25,000  
Location & Darkness Fairvale Observatory – Redhill – Surrey – UK        Typically Bortle 5
Date & Time 5h + 6th + 7th  May 2018 @ 23.30h  approx.

 

 

Death Throes of a Star

Abell 21 RGB 1Final (Large)

As the winter arm of the Milky Way proceeds inexorably towards the west, I’ve been seeking new objects and was pleasantly surprised to recently discover a small but nonetheless interesting planetary nebula located just to the east of the galactic plane between Canis Minor and Gemini.  Consisting of large filaments of glowing ionized gas, the feature goes by the popular name of the Medusa Nebula, after the Greek mythological gorgon figure which has hair of writhing snakes!

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Statue of Medusa

Also known as Abell 21 (discovered by George Abell in 1955), Medusa is an ancient planetary nebula some 1,500 light-years away, officially situated within the constellation Gemini.  Like its dramatic mythological namesake, the planetary nebula represents the final stages of a low mass star such as our sun in the process of transforming from a red giant to hot a white dwarf star, in the process shedding its outer layers which are illuminated by ultraviolet radiation from the hot star within which powers its glow.

Medusa

At 4-light years across the Medusa Nebula is a small though reasonable size but with an apparent magnitude of some +15.99 is very faint and is therefore difficult to image.  Nonetheless, Ha and OIII gases are prevalent and as something of an experiment I chose to try and image this object at narrowband wavelenghts.

Abell 21 RGB 1FinalCrop (Large)

Considering the aforesaid problems I am quite pleased with the outcome (top of page), indeed I was surprised to see I had captured anything.  However, given its challenging low brightness and a total integration time of only 75-minutes, the final image was always going to be lacking in detail and noisy (cropped image immediately above).  Notwithstanding, now I know of its presence I will surely be returning to The Medusa Nebula on another occasion to improve the integration time and perhaps use a larger telescope to grab those photons which prove elusive to my current equipment set-up.

 

IMAGING DETAILS
Object The Medusa Nebula    (Abell 21 / Sharpless 2-274)     
Constellation Gemini
Distance 1,500 light-years
Size Approx. 12’ x 9’
Apparent Magnitude +15.99
 
Scope  William Optics GT81 + Focal Reducer FL 382mm  f4.72
Mount SW AZ-EQ6 GT + EQASCOM computer control
Guiding William Optics 50mm guide scope
  + Starlight Xpress Lodestar X2 guide camera & PHD2 control
Camera ZWO1600MM-Cool (mono)   CMOS sensor
  FOV 2.65o x 2.0o    Resolution 2.05”/pix  Max. image size 4,656 x 3,520 pix   
EFW ZWOx8 + ZWO LRGB & Ha OIII SII 7nm filters 
Capture & Processing Astro Photography Tool,  Deep Sky Stacker & Photoshop CS2
Exposures 10 x 300 sec Ha, 5 x 300 sec  OIII   (Total time: 75 minutes)
  @ 139 Gain  21 Offset @ -20oC  
Calibration 5 x 300 sec Darks  20 x 1/4000 sec Bias  10 x Flats Ha, OIII & SII @ ADU 25,000  
Location & Darkness Fairvale Observatory – Redhill – Surrey – UK        Typically Bortle 5
Date & Time 11th February 2018 @ 23.00h approx.

 

The Fox & Cone

Cone Ha100 20 15 OIII B CROP

After the fun of December and January provided by the wide choice of exciting DSO objects, February affords a worthy finale to the winter season, in particular within the constellation Monoceros.  After successfully imaging the Rosette Nebula on 9th February, a few days later I was able to move on to another nearby HII-region in the Milky Way, with equally good results.  Surprisingly it’s been just over 3-years since I last imaged the same part of the sky just before Christmas 2014, on that occasion with an unmodded Cannon 700D DSLR.  Now armed with the more capable ZWO1600MM-Cool camera and narrowband filters, the potential for raising the bar was good and the results did not disappoint.

Untitled

Of foremost interest this time was NGC 2264, which officially describes the Cone Nebula and Christmas Tree Cluster but also includes the Snowflake Cluster and Fox Fur Nebula, all set within a large HII-region.  Individually each object is towards the limit of my equipment’s resolution but taken all together makes for an interesting combination when encompassed inside the 2.65o x 2.00o field-of-view.  Like the Rosette I chose to image in narrowband, with a total integration time of 90 minutes; again using 300 second subs at Unity gain proved to be very effective – I suspect that only more subs rather than longer exposures would lead to a better outcome but that will have to wait until I’ve sorted how to plate solve, watch this space!

Picture saved with settings embedded.

I’ve recently been experimenting in Photoshop using star masks and related sharpening and contrast enhancement methods, which for the first time I applied when processing these images to great effect.   Being an HII-region the overall image area is dominated by Ha-light and the processed Ha-subs resulted in a very exciting image at this wavelength, with many subtleties revealed throughout (see below).  On the other hand OIII and especially SII wavelengths are much less prevalent, from which it would seem  that a higher ratio of those subs would be required to better tease out detail at those wavelengths.  Notwithstanding, the resulting Ha-OIII-OIII Bi-Colour image has turned out well (top of the page), with all the aforementioned objects showing clearly.

Picture saved with settings embedded.

The signature object of this image is probably the Cone Nebula.  New stars are forming within a cone shaped dark molecular cloud, itself sculpted by strong stellar winds. However, I consider the Fox Fur Nebula (Sharpless-273) to be the bigger imaging challenge, which I’m therefore pleased to say is starting to show well in these images.  The name derives from the rich, fur-like texture of the nebula which is also shaped by stellar winds; reckon The Fox & Cone would make a good pub name! Below:  Cone Nebula & Christmas Tree Cluster Ha-OIII-OIII before colour mapping.

Cone Ha100 20 15 OIII A crop

But there’s more. A series of stars form an inverted outline shape of the so-called Christmas Tree Cluster above the Cone Nebula (see image above), with the conspicuously bright 15 Monocerotis at its base made of a massive variable star system.  And finally, somewhat off piste, lurking in the top right corner of the main image is NGC 2261 or Hubble’s Variable Nebula.  Discovered by Edwin Hubble in 1949, the nebula is illuminated by the unseen R Monocerotis star and forms a small but distinct bright triangular area.

All-in-all this is a great part of the February sky for imaging.  There’s still more to discover and I won’t leave it as long as 3-years before going back again, with the objectives of increasing integration time and possible addition of RGB subs to enhance the colour potential.

IMAGING DETAILS
Object Fox  & Cone Nebulae  NGC 2264 + Hubble’s Variable Nebula NGC  2261     
Constellation Monoceros
Distance 2,700 light-years
Size Approx. 54’ x 37’
Apparent Magnitude +3.9
 
Scope  William Optics GT81 + Focal Reducer FL 382mm  f4.72
Mount SW AZ-EQ6 GT + EQASCOM computer control
Guiding William Optics 50mm guide scope
  + Starlight Xpress Lodestar X2 guide camera & PHD2 control
Camera ZWO1600MM-Cool (mono)   CMOS sensor
  FOV 2.65o x 2.0o    Resolution 2.05”/pix   Max. image size 4,656 x 3,520 pix   
EFW ZWOx8 + ZWO LRGB & Ha OIII SII 7nm filters 
Capture & Processing Astro Photography Tool,  Deep Sky Stacker & Photoshop CS2
Exposures 12 x 300 sec Ha, 6 x 300 sec  OIII   (Total time: 90 minutes)
  @ 139 Gain  21 Offset @ -20oC  
Calibration 5 x 300 sec Darks  20 x 1/4000 sec Bias  10 x Flats Ha, OIII & SII @ ADU 25,000  
Location & Darkness Fairvale Observatory – Redhill – Surrey – UK        Typically Bortle 5
Date & Time 11th February 2018 @ 21.00h

What Comes Around Goes Around

RGB HaOO XXX2

It’s nearly 4-years since I started astronomy, like so many inspired after observing Saturn through a telescope.  Not just any telescope but the 13” Astrographic Refractor at the Observatory Science Centre in Herstmonceaux.  Built in 1890 specifically to make use of the then new technique of astrophotography, the telescope was first employed as part of the worldwide Carte Du Ciel project to map the entire night sky by photography and subsequently for a crucial test of Einstein’s then new theory of General Relativity.  Soon thereafter I was to view the aforesaid planet once again with my first, newly purchased Skywatcher 150PL Newtonian telescope.  Inevitably something of a lesser view than that at Herstmonceaux it was nonetheless just as exciting, if not more so.  I was hooked!

I then attempted afocal imaging using a compact camera held up to the telescope eyepiece but with poor results, except in one respect.  By clamping the camera onto the front of the eyepiece and achieving longer exposures, nebulosity otherwise unseen with the naked eye was revealed in the resulting image, in this case Orion’s Nebula.  As crude as the image was, for me the penny had dropped and I’ve been pursuing images of the hidden beauty of the night sky ever since.

rosette map

ngc2237map

Like mariners, through astronomy I have by now become accustomed to the seasonal procession of the night sky wonders throughout the year, none more so than the Rosette Nebula.  About 100 light-years across and 5,000 light-years from Earth, the Rosette Nebula is surely one of the annual highlights for most astrophotographers?  Located just east of Orion, the Rosette is at its best between December and February, so that I was first able to image this beautiful object myself at the end of 2014.

As a very large HII region the Rosette Nebula emits light mainly at narrowband wavelengths, which produces wonderful but mainly red colours when imaged with a modded DSLR camera.  As my astrophotography and equipment have since developed, it has become a pleasure and challenge to image objects as they return each year such as the Rosette, thereby also charting my own improvements or otherwise from year-to-year.  Its size makes the Rosette an especially attractive target for smaller telescopes such my own with an 81mm aperture, which nicely fills much of the sensor of an APS-C camera.

Despite having purchased a new ZWO1600MM-Cool mono camera at the end of 2016, by the time I was ready to use it at the end of the following March, the Rosette Nebula had almost disappeared over the western horizon for another year.  Notwithstanding, in the limited time remaining I managed to capture a few Ha-OIII-SII subs, thus marking first light for the camera, which ironically resulted in one of my favourite images for 2017.  Using narrowband for the first time it was immediately possible to see the potential of the new camera when imaging this type of object.

Returning from an extended overseas trip at the end of January this year, 10-months had passed since my last encounter with the Rosette Nebula last March and I found myself with the first real opportunity to image the nebula properly with the ZWO1600MM-Cool camera.  Since last year I’d acquired more knowledge and experience with the camera, plus this time the Rosette was now in the south eastern quadrant and provided significantly more imaging time than before.

After a break of nearly two months I needed to sort out the equipment, refocus the camera and start a new alignment model in EQASCOM.  For the first time I also decided to use longer exposure times of 300 seconds, which altogether produced a good Ha+OIII Bi-Colour image (top of page – awarded BAA Picture of the Week 4th March 2018); whilst much longer exposures are used with conventional CCD sensors, such is the sensitivity of the CMOS mono sensor in the ZWO camera that 5-minute exposures provide exceptionally good quality data.  Overall the impact of longer exposure, good focus, tracking and much longer total integration time had a noticeably positive impact on noise and overall image quality, though there’s still room for improvement – there always is!

To some extent, even after a year I’m still in the experimental phase with this camera.  For most of 2017 I used a high gain setting of 300 but this time I chose the Unity gain setting of 139 and for interest also imaged at a shorter exposure of 180 seconds.  Comparison between the two settings for Ha images – Unity gain at 300 and 180 seconds – shows that for such a nebulous type of feature as the Rosette, Unity gain works very well at the longer 300 second exposure (first image below) but not 180 seconds (second image below), which is too short to collect sufficient data.

Picture saved with settings embedded.

Picture saved with settings embedded.

Notwithstanding, in the past I have found shorter exposures at Unity or less have generally been more suitable for brighter objects such as star clusters or galaxies like Andromeda.  An alternative SHO Hubble Palette image below of the Rosette Nebula at Unity gain and 300 second exposure also compares more favourably with the same image taken last year using less subs, higher gain and shorter exposure time.

Untitled-2 Crop2 (Large)When the object is right, such as the Rosette Nebula, narrowband imaging using the ZWO camera produces exceptional results.  This is evident in these recent images where it’s now possible to clearly see structural elements of the nebula, as well as the star fields located within.  Frankly I am very excited by these new images and can’t wait for next year to come around again!

Postscript: Research at Leeds University just published suggests that the Rosette Nebula is a disc but I believe my eyes and this image and many others which says otherwise!

IMAGING DETAILS
Object Rosette Nebula     NGC 2244 + 2237, 2238, 2239 & 2246   
Constellation Monoceros
Distance 5,000 light-years
Size Approx. 100 light-years or 1.3o
Apparent Magnitude +9.0
 
Scope  William Optics GT81 + Focal Reducer FL 382mm  f4.72
Mount SW AZ-EQ6 GT + EQASCOM computer control
Guiding William Optics 50mm guide scope
  + Starlight Xpress Lodestar X2 guide camera & PHD2 control
Camera ZWO1600MM-Cool (mono)   CMOS sensor
  FOV 2.65o x 2.0o    Resolution 2.05”/pix   Max. image size 4,656 x 3,520 pix   
EFW ZWOx8 + ZWO LRGB & Ha OIII SII 7nm filters 
Capture & Processing Astro Photography Tool,  Deep Sky Stacker & Photoshop CS2
Exposures 12 x 300 sec Ha, 6 x 300 sec  OIII & SII  (Total time: 120 minutes)
  @ 139 Gain  21 Offset @ -20oC  
Calibration 5 x 300 sec Darks  20 x 1/4000 sec Bias  10 x Flats Ha, OIII & SII @ ADU 25,000  
Location & Darkness Fairvale Observatory – Redhill – Surrey – UK        Typically Bortle 5
Date & Time 9th February 2018 @ 22.00h

 

Antipodean Astronomy Adventures

IMG_9050 (Large)

I’ve recently returned from visiting family on an extended trip to Aotearoa – Maori for New Zealand – and whilst travelling around used the opportunity to learn something about astronomy in that part of the world (NZ Astro Directory).  Of course, the main difference Down Under is that it’s currently summer, plus everything in the night sky is upside down.

IMG_0003crop anotate

Topsy Turvy – everything’s in the wrong place ! Red arrow = Betelgeuse, Yellow arrow = Orion Nebula

It’s obvious really but relatively speaking the sky has not changed, you’re just  personally inverted compared to the Northern Hemisphere – which from the point of view of astronomy takes some getting used to when looking at otherwise familiar objects such as the Moon or Orion Constellation.  Although being their summer, at our principal location of latitude of 38o on North Island there was more than four hours of astronomical darkness even on the December solstice; viewed from the perspective of the Northern hemisphere, it is interesting to note that this is about the same latitude as Athens or the Korean DMZ!

Moon Man

It’s all about perspective – obvious really!

Although the weather was mostly very good, I was struck by how frequently the sky at night was cloudy – just like good old Blighty – it is after all also known as The Land of the Long White Cloud by the Maori.  Notwithstanding, as a country with only 4.85 million people most of the country is rural or even desolate, so that when the skies are clear the darkness and seeing conditions can be quite spectacular.  Viewing conditions are particularly good on South Island around the Lake Tekapo and Mt Cook district where a number of astronomy ventures are based, including the University of Canterbury’s Mt John Observatory – shown at the beginning of this blog.  For practical reasons I was restricted to taking only limited equipment – DSLR & lenses + Gorilla Pod & ball head + Vixen Polarie tracker + 10×50 binoculars – but was still able to obtain some pleasing images during the trip.

IMG_9081 (Large)

Mt Cook from near our campsite – the night sky here was fantastic

Early on it became evident that New Zealand seems to have all the right conditions required for the formation of lenticular clouds (altocumulus lenticularis).  I’m presuming this is related to its somewhat exposed position between the South Pacific Ocean and Tasman Sea, thus providing favourable wind and moisture conditions which are then influenced by the mountainous tectonic terrain that runs along the spine of South Island and the volcanic topography of North Island.  Whatever it is it works, providing really beautiful and often spectacular sights of these elusive and somewhat rare high altitude cloud phenomena.

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Lenticular clouds south of Mt Cook – South Island 

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Lenticular clouds near Te Awamutu – North Island 

Prior to arriving in New Zealand I tried unsuccessfully to link up with some local astronomy clubs.  However, close to our base near Te Awamutu on North Island I was able to visit the Te Awamutu Space Centre at nearby Kihikihi.

IMG_20180115_130500614

The Te Awamutu Space Centre – Kihikihi

Conceived and run by the enthusiastic Brit Dave Owen (well he wasn’t going to be a Kiwi was he?), the Centre is an eclectic and interesting collection of space, space programme, astronomy and related educational items (see below).

Essentially the Centre is an outreach programme, which would be of interest to anyone in general, young and old, as well as the seasoned astronomer.  I particularly found the area on New Zealand astronomy & astronomers, astronauts and the historical role of Maoris in astronomy very  interesting.

Pliades

Maori star names of Mataraki (Pleiades)

As we travelled the length and breadth of the country with the tantalising promise of some very dark skies, I was keen to view and image the Milky Way and particularly the Large and Small Magellanic Clouds, which are only visible from the Southern Hemisphere. Thwarted for a while by cloud cover I eventually got my first look at all these features whilst camping near the base of the 3,724 metre Mt Cook on South Island.  The sight did not disappoint but I was unfortunately unable to obtain any images on this occasion.

No worries (as they say in New Zealand – frequently!), a few nights later whilst camping at the improbably named Slab Hut Creek (site of old alluvial gold workings) west of the historic mining town of Reefton, I was at last able to image all these features.  Remotely situated in the middle of woods adjacent to the aforesaid gold creek, the night sky was inky black, albeit with some passing cloud from time-to-time.  Furthermore, located in the centre of the opening were two very large quartz boulders, which provided an ideal platform on which to set up the camera and Gorilla Pod.

IMG_9280 (Large)

A few tons of conveniently placed quartz helped imaging later in the night!

I didn’t get much sleep that night but it was a magical experience and I was thrilled to image both the Milky Way and Magellanic Clouds not individually but together.  As an added bonus we were also able to successfully undertake some gold panning during the day in the creek!

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The Milky Way at Slab Hut Creek with the Large & Small Magellanic Clouds

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Thereafter I was hindered for the next few weeks by Christmas events and the inevitable full moon at the start of January, though the ISS did pass directly overhead on one evening (New Zealand from the ISS).  However, 10-days later back on North Island at our cottage in the Waipa district, I was eventually able to view and image once again the wonderful sight of the Milky Way + Magellanic Clouds + Southern Cross at the same time – sky chart and image below.

Ohaupo Sky

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From our base on North Island: The Milky Way & Magellanic Clouds (right) + Southern Cross just above the left-hand side of the roof line 

When the conditions are right the night sky in New Zealand is truly outstanding. I would have liked to spend time there with the full astronomy set-up and camera that I use in the UK but for now I was very pleased to experience and enjoy Antipodean astronomy, it really is worth the long journey.